Optimizing the analysis of emission lines in galaxies: the case of the MUSE TIMER galaxy NGC 613
Galaxy evolution is driven by spatially distributed processes with varying time-scales. Integral field spectroscopy provides spatially resolved information about these processes. Nevertheless, disentangling these processes, which are related to both the underlying stellar populations and the interstellar medium can be challenging. We present a case
Silva-Lima, Luiz A. et al.
Fecha de publicación:
7
2025